地球与空间科学 · 第 3 册 · 本科一年级

University Earth and Space Sciences — Year 1

书籍暂未推出简体中文版——当前显示英文版。

University Earth and Space Sciences — Year 1 · 本科一年级

13Rifts, Ridges and Passive Margins

In September 2005 the ground of the Afar desert, in the north-east of Ethiopia, opened. Within three weeks a stretch of the rift some 60 km60\,\mathrm{km} long widened by up to 8 m8\,\mathrm{m}, and about 2.5 km32.5\,\mathrm{km}^{3} of magma rose into the crack from below. The plates there separate at about 18 mm18\,\mathrm{mm} a year: the crisis released, in a few weeks, the stretching of some four centuries. Afar is a continent breaking apart; a few hundred kilometres to the north, the Red Sea is a young ocean whose floor is already made like the floor of the Atlantic, and the South Atlantic was such a rift before it opened, about 120 million years ago. This chapter follows the birth of an ocean: the stretching of a continent, its break-up, the two passive margins left behind, the ridge that builds the ocean floor, and the slow sinking of that floor as it cools.

You already know

The plates are the upper thermal boundary layer of the mantle; under the oceans a cooling half-space describes them, and their isotherms deepen as the square root of age (Chapter 10). Columns of rock in isostatic equilibrium have the same mass per unit area above a compensation depth (Chapter 11). Plates turn about Euler poles, ridges spread at rates read from magnetic anomalies, and transforms lie on small circles about the pole (Chapter 12). The throw and the heave of a fault were defined in Chapter 5; a normal fault is an inclined fault whose upper block has moved down (Book 2, grade 11).

13.1 Continental rifting

A continent stretched by forces at its edges does not thin evenly. Its brittle upper crust breaks along normal faults, and the blocks between them sink and tilt; below, the warmer lower crust and the mantle flow.

Definition 13.1 (Continental rift, graben, half-graben)

A continental rift is a long, narrow zone where a continent is being stretched: a depression bounded by normal faults, with earthquakes and, often, volcanoes. A graben is a block dropped between two normal faults that dip towards each other. A half-graben is a block dropped and tilted against a single major normal fault, the border fault, on one side only.

Most rift basins are chains of half-grabens. Their border faults hand the displacement over to one another through relay ramps, and the side of the border fault often alternates from one segment to the next. The hanging wall of each border fault tilts down towards it, and the basin fills fastest there: the thickest sediment piles up against the fault, while the footwall is raised into the rift shoulder.

The horizontal stretching carried by a fault is its heave. A planar normal fault of throw hh and dip δ\delta has the heave h/tan⁡δh/\tan\delta (Chapter 5); adding the heaves of the faults across a rift section gives the extension of the brittle crust. How the whole lithosphere thins as it is stretched, and why it then subsides, is quantified in the Year 2 volume; here the faults are measured, and their sum compared with the motion of the plates.

An open fissure in the lava floor of the Þingvellir rift valley, in south-west Iceland, where the Mid-Atlantic Ridge comes ashore. The basalt flows of the valley floor are cut by open fissures parallel to the rift. Photograph: Olga Ernst, CC BY-SA 4.0 (Wikimedia Commons).
An open fissure in the lava floor of the Þingvellir rift valley, in south-west Iceland, where the Mid-Atlantic Ridge comes ashore. The basalt flows of the valley floor are cut by open fissures parallel to the rift. Photograph: Olga Ernst, CC BY-SA 4.0 (Wikimedia Commons).

Volcanic and magma-poor rifts

Rifts differ in how much magma they receive. In a magma-poor rift the stretching is taken up by faults, and the crust thins as the blocks slide apart. In a volcanic rift magma takes over: dykes intrude the crust along the axis, each one opening the rift by its own thickness, and lavas flood the surface. The East African Rift shows both, side by side: its eastern branch is strongly volcanic, while its western branch is less so and holds deep sedimentary basins, filled by lakes such as Lake Tanganyika and bounded by faults.

Both branches began to form about 25 million years ago, and the rift splits the African plate into a Nubian plate to the west and a Somali plate to the east. From the Afar triple junction it runs south, in two branches around the old, thick and cold Tanzania craton. Its motion is slow: computed from the plate vectors of Somalia and Nubia, each measured relative to the Antarctic plate, Somalia moves away from Nubia at 6.0 mm yr−16.0\,\mathrm{mm}\,\mathrm{yr}^{-1} towards 105∘105{}^{\circ} in central Ethiopia (8.5∘8.5{}^{\circ} N, 39.5∘39.5{}^{\circ} E), and at 5.1 mm yr−15.1\,\mathrm{mm}\,\mathrm{yr}^{-1} on the equator. Many earthquakes of the rift show normal faulting.

In Afar, at the northern end, the rift meets the Red Sea and the Gulf of Aden. The bulk of the Ethiopian flood basalts erupted there about 30 million years ago, in a million years or less, and magma has kept arriving since: lava flows at the surface, intrusions in the crust and new material added below it, so much that the intruded crust has kept its thickness through the early stages of rifting. The crisis of 2005 shows how such a rift opens: not steadily, but in episodes, each a dyke metres wide intruded within days or weeks. Since the plates diverge at about 18 mm yr−118\,\mathrm{mm}\,\mathrm{yr}^{-1} there, the 8 m8\,\mathrm{m} dyke of 2005 took up the stretching of about 440 years.

13.2 Break-up and passive margins

If stretching goes on, the continental crust is thinned to nothing, the mantle rises beneath the rift and melts as it rises, and the first oceanic crust forms between the two halves of the continent. That moment is the break-up. From then on the plates move apart at a ridge in the middle of a new ocean, and the two edges of the continent, carried away from the ridge, stop being plate boundaries.

Definition 13.2 (Passive margin, ocean–continent transition, break-up unconformity)

A passive margin is the edge of a continent that was formed by rifting and is no longer a plate boundary: the continent and the adjacent ocean floor belong to the same plate. The ocean–continent transition is the zone of the margin, kilometres to tens of kilometres wide, between thinned continental crust and normal oceanic crust. The break-up unconformity is the unconformity that separates the sediments deposited in the rift basins, tilted with their blocks, from the undisturbed sediments laid over the margin after break-up.

Passive margins line most of the Atlantic, the Arctic Ocean and the western Indian Ocean, and nearly all the coasts of Africa, Australia, Greenland and India. The eastern margin of North America and the north-western margin of Africa were the two sides of one rift: they are conjugate margins. Their profile is the familiar sequence of the ocean floor near land: continental shelf, slope, rise and abyssal plain. Under the shelf and slope lies the thinned continental crust, cut by normal faults that dip towards the ocean, with its rotated blocks buried beneath the sediments.

From rift to passive margin (drawings, not to scale; the heights are exaggerated). (a) The brittle upper crust breaks along normal faults; blocks tilt into half-grabens that fill with sediment, and the Moho rises under the thinned crust. (b) At break-up the continental crust is cut through; the sea floods the rift and the first oceanic crust forms. (c) One of the two margins, carried away from the ridge: its tilted blocks and their sediments lie under the break-up unconformity, buried by the post-rift sediments of the shelf, slope and rise.
From rift to passive margin (drawings, not to scale; the heights are exaggerated). (a) The brittle upper crust breaks along normal faults; blocks tilt into half-grabens that fill with sediment, and the Moho rises under the thinned crust. (b) At break-up the continental crust is cut through; the sea floods the rift and the first oceanic crust forms. (c) One of the two margins, carried away from the ridge: its tilted blocks and their sediments lie under the break-up unconformity, buried by the post-rift sediments of the shelf, slope and rise.

Two kinds of margin

Margins inherit the character of their rift. On magma-poor margins, such as those of Iberia and Newfoundland, the seismic sections show rotated blocks whose beds dip towards the continent; in places the ocean–continent transition is floored by mantle peridotite, brought up to the sea floor and altered by sea water to serpentinite. On volcanic margins, such as the mid-Norwegian, East Greenland, Namibian and Brazilian margins, the transition is built of basalt: stacks of lava flows that dip towards the ocean, the seaward-dipping reflectors of seismic sections, and below them a lower crust in which P waves travel unusually fast, magma added beneath the crust at break-up. Volcanic margins subside little during break-up.

In the field — Finding the edge of a continent

The ocean–continent transition lies under kilometres of water and sediment, and is located only by geophysics, usually by several methods together. Seismic reflection images the tilted blocks, the break-up unconformity and, where the signal reaches deep enough, the Moho. Wide-angle seismic refraction measures the speeds of P waves through the crust, which differ between continental and oceanic crust. Gravity data, inverted for the depth of the Moho, give the thickness of the crust. The magnetic stripes of the ocean floor stop where the continental crust, magnetically quiet, begins.

After break-up a margin sinks. During rifting the lithosphere was thinned and heated; carried away from the ridge, it cools and contracts, like the ocean floor beside it, and the space that opens above it fills with the wedge of post-rift sediments, whose weight presses it down further. The cooling half of this story is told in Section 13.4; the weight of the sediments is the subject of Chapter 23.

13.3 Fast and slow ridges

Once the ocean is born, it grows at its ridge. Ridges spread at very different rates: the rates measured over the last few million years run from 9.7 mm yr−19.7\,\mathrm{mm}\,\mathrm{yr}^{-1} in the northern Red Sea to 154.4 mm yr−1154.4\,\mathrm{mm}\,\mathrm{yr}^{-1} on the East Pacific Rise. Their shape depends on that rate.

Definition 13.3 (Fast-, slow- and ultraslow-spreading ridges)

A ridge is classed by its full spreading rate. An ultraslow-spreading ridge opens at less than about 20 mm yr−120\,\mathrm{mm}\,\mathrm{yr}^{-1}; a slow-spreading ridge at 20 to 55 mm yr−155\,\mathrm{mm}\,\mathrm{yr}^{-1}; an intermediate ridge at 55 to 75 mm yr−175\,\mathrm{mm}\,\mathrm{yr}^{-1}; a fast-spreading ridge at more than about 75 mm yr−175\,\mathrm{mm}\,\mathrm{yr}^{-1}.

The limits are conventions and vary between authors. What does not vary is the change of form. A slow ridge, such as the Mid-Atlantic Ridge, has an axial valley between inward-facing normal faults: the gap between the plates is not filled by magma as fast as it opens, and the cold lithosphere breaks. A fast ridge, such as the East Pacific Rise, has no rift valley but a smooth axial high over a lens of melt, refilled often enough to keep pace. Either way the axis lies about 2500 m2500\,\mathrm{m} deep, and the oldest floor of the basins nearly 4 km4\,\mathrm{km} deeper (Section 13.4).

Ultraslow ridges show what happens when magma is scarcest: their volcanism is intermittent, they lack transform faults, and over large regions the mantle itself is brought up to the sea floor. The Gakkel Ridge, under the Arctic Ocean, the slowest of all, is not offset at all; along a central stretch of its axis some 300 km300\,\mathrm{km} long, mantle peridotite lies directly on the axis, between abundant volcanism to the west and large, widely spaced volcanoes to the east. On slow and ultraslow ridges especially, part of the spreading is taken up by long, gently dipping normal faults, detachments, whose footwall is pulled out from under the axis: gabbro and peridotite reach the sea floor in corrugated domes, oceanic core complexes. The Atlantis Massif, beside the Mid-Atlantic Ridge near 30∘30{}^{\circ} N, is one: on its top, on crust 1.5 Myr1.5\,\mathrm{Myr} old about 15 km15\,\mathrm{km} from the axis, sea water reacting with the mantle rock feeds the warm, alkaline springs of the Lost City hydrothermal field.

The oceanic crust

Definition 13.4 (Oceanic crust, pillow lava, sheeted dyke complex)

The oceanic crust is the crust made at ocean ridges: 6 to 7 km7\,\mathrm{km} of basalt and gabbro, from the sea floor down to the Moho, beneath a cover of sediments. Pillow lava is lava erupted under water, made of rounded, interconnected tubes and lobes, each with a glassy skin chilled by the sea. A sheeted dyke complex is a layer made almost entirely of parallel vertical dykes, each intruded into the previous ones.

The layers of the oceanic crust were first defined by seismology, then sampled by drilling and recognised in slices of ocean floor thrust onto continents, the ophiolites. From the top:

  • layer 1, sediments, thin or absent near the ridge and thickening with the age of the floor;
  • layer 2, on average 1.84 km1.84\,\mathrm{km} of basalt: pillow lava at the top (layer 2A), sheeted dykes of diabase below (layer 2B);
  • layer 3, the remaining four to five kilometres, of gabbro and, at its base, cumulates settled from the magma: some 70 %70\,\% of the thickness of the crust.

Beneath the Moho lies mantle peridotite, the residue left by the melting.

Seismic refraction gives the igneous crust a mean thickness of (7.1±0.8) km(7.1 \pm 0.8)\,\mathrm{km} away from fracture zones and hot spots, and a later synthesis of seismic profiles 6.15 km6.15\,\mathrm{km}, much the same at all spreading rates: the amount of melt depends on the temperature of the rising mantle, not on the speed at which it rises. Only very slow ridges make anomalously thin crust: the mantle there has time to cool as it rises, and melts less. Over a hot plume the crust is thicker, about 20 km20\,\mathrm{km} directly above the rising core of a plume, as under Iceland (Chapter 15). Along all the ridges together, about 3.0 km23.0\,\mathrm{km}^{2} of new sea floor and some 20 km320\,\mathrm{km}^{3} of new crust are made each year.

Pillow lavas on the Galápagos Rift, cut by a fissure that opened after they had set: the top of layer 2 of the oceanic crust as it forms. Each pillow is a tongue of lava frozen from the outside by the sea water. Photograph: NOAA Okeanos Explorer Program, Galápagos Rift Expedition 2011, CC BY 2.0 (Wikimedia Commons).
Pillow lavas on the Galápagos Rift, cut by a fissure that opened after they had set: the top of layer 2 of the oceanic crust as it forms. Each pillow is a tongue of lava frozen from the outside by the sea water. Photograph: NOAA Okeanos Explorer Program, Galápagos Rift Expedition 2011, CC BY 2.0 (Wikimedia Commons).

Proposition 13.5 (Each dyke splits the one before)

Suppose that every dyke of a sheeted dyke complex is intruded along the axis of spreading, where the crust is hottest and weakest, and that the crust moves away from the axis symmetrically. Then most dykes are found split in two, each half with a chilled margin against its older neighbour only.

Proof. A dyke chills against the colder rock on both sides: it has two chilled margins when it forms. The next dyke rises where the crust is weakest, along the axis, that is, through the middle of the previous one, still the hottest rock. It splits it into two halves, which the spreading carries away on either side; each half keeps the chilled margin on its outer side and has, on its inner side, the uncooled contact with the new dyke. Every dyke but the last is split in this way. ∎

Dykes with a chilled margin on one side only are indeed the rule in sheeted dyke complexes: the signature of a crust built, dyke after dyke, by spreading.

13.4 The depth–age law

Ocean floor is shallow at the ridge and deep far from it. Since floor is made at the ridge and carried away, distance from the ridge is age, and the depth of the floor depends on its age. The plate cools from above as it ages (Chapter 10); cold rock is denser, and a denser column floats lower.

Lemma 13.6 (An integral of the error function)

With erfc⁡u=1−erf⁡u=2π∫u∞e−s2 ds\operatorname{erfc} u = 1 - \operatorname{erf} u = \frac{2}{\sqrt\pi}\int_u^\infty e^{-s^2}\,\mathrm ds,

∫0∞erfc⁡u du=1π.\int_0^\infty \operatorname{erfc} u \,\mathrm du = \frac{1}{\sqrt\pi}.

Proof. The derivative of erfc⁡\operatorname{erfc} is −2πe−u2-\frac{2}{\sqrt\pi}e^{-u^2}. Integrating by parts on [0,X][0, X],

∫0Xerfc⁡u du=[uerfc⁡u]0X+2π∫0Xu e−u2 du=Xerfc⁡X+1π(1−e−X2).\int_0^X \operatorname{erfc} u\,\mathrm du = \bigl[u \operatorname{erfc} u\bigr]_0^X + \frac{2}{\sqrt\pi}\int_0^X u\,e^{-u^2}\,\mathrm du = X\operatorname{erfc} X + \frac{1}{\sqrt\pi}\bigl(1 - e^{-X^2}\bigr).

For X>0X > 0 and s≥Xs \ge X, e−s2≤(s/X)e−s2e^{-s^2} \le (s/X)e^{-s^2}, so Xerfc⁡X≤2π∫X∞s e−s2 ds=e−X2/πX\operatorname{erfc} X \le \frac{2}{\sqrt\pi}\int_X^\infty s\,e^{-s^2}\,\mathrm ds = e^{-X^2}/\sqrt\pi, which tends to 0. Letting X→∞X \to \infty gives the result. ∎

Theorem 13.7 (Depth–age law)

Suppose that

  1. the mantle leaves the ridge at the uniform temperature TmT_m, and the oceanic plate of age tt is a half-space cooled since then from its surface, held at T0T_0, with the thermal diffusivity κ\kappa;
  2. the density of the cooled rock is ρm(1+α(Tm−T))\rho_m\bigl(1 + \alpha(T_m - T)\bigr), with ρm\rho_m the density of the mantle at TmT_m and α\alpha its coefficient of thermal expansion;
  3. every column is in isostatic equilibrium above a compensation depth lying below the cooled layer, and sea water has the density ρw\rho_w.

Then the depth of the sea floor of age tt is

d(t)=dr+Ct,C=2π ρm α (Tm−T0)κρm−ρw,d(t) = d_r + C\sqrt t, \qquad C = \frac{2}{\sqrt\pi}\,\frac{\rho_m\,\alpha\,(T_m - T_0)\sqrt\kappa}{\rho_m - \rho_w},

where drd_r is the depth of the ridge axis. This is the depth–age law of the ocean floor.

Proof. The temperature in the cooled half-space is

T(z,t)=T0+(Tm−T0)erf⁡z2κt,T(z, t) = T_0 + (T_m - T_0)\operatorname{erf}\frac{z}{2\sqrt{\kappa t}},

with zz the depth below the sea floor; this solution of the heat equation is admitted here, as in Chapter 10, and derived in the Year 3 volume. Compare the column at the ridge, made of water down to drd_r and of mantle at TmT_m below, with the column of age tt, made of water down to dd and of the cooled plate below, both down to the compensation depth DD. Their masses per unit area are equal:

ρwdr+ρm(D−dr)=ρwd+∫0D−dρm(1+α(Tm−T))dz=ρwd+ρm(D−d)+ρmα∫0D−d(Tm−T) dz.\rho_w d_r + \rho_m (D - d_r) = \rho_w d + \int_0^{D-d}\rho_m\bigl(1 + \alpha(T_m - T)\bigr)\mathrm dz = \rho_w d + \rho_m (D - d) + \rho_m\alpha\int_0^{D-d}(T_m - T)\,\mathrm dz.

Hence

(ρm−ρw)(d−dr)=ρmα∫0D−d(Tm−T) dz.(\rho_m - \rho_w)(d - d_r) = \rho_m\alpha\int_0^{D-d}(T_m - T)\,\mathrm dz.

Since Tm−T=(Tm−T0)erfc⁡(z/2κt)T_m - T = (T_m - T_0)\operatorname{erfc}\bigl(z/2\sqrt{\kappa t}\bigr) is negligible below the cooled layer, the integral may be taken to infinity; with u=z/2κtu = z/2\sqrt{\kappa t} and Lemma 13.6,

∫0∞(Tm−T) dz=(Tm−T0) 2κt∫0∞erfc⁡u du=2π(Tm−T0)κt.\int_0^\infty (T_m - T)\,\mathrm dz = (T_m - T_0)\,2\sqrt{\kappa t}\int_0^\infty\operatorname{erfc}u\,\mathrm du = \frac{2}{\sqrt\pi}(T_m - T_0)\sqrt{\kappa t}.

Dividing by ρm−ρw\rho_m - \rho_w gives d−dr=Ctd - d_r = C\sqrt t. ∎

The water matters: as the plate sinks, water fills the space above it, and its weight presses the plate further down. The effective expansion coefficient αρm/(ρm−ρw)\alpha\rho_m/(\rho_m - \rho_w) is larger than α\alpha by the factor 3300/2300≈1.433300/2300 \approx 1.43.

With α=3.2×10−5 K−1\alpha = 3.2 \times 10^{-5}\,\mathrm{K}^{-1}, Tm−T0=1350 KT_m - T_0 = 1350\,\mathrm{K}, κ=10−6 m2 s−1\kappa = 10^{-6}\,\mathrm{m}^{2}\,\mathrm{s}^{-1}, ρm=3300 kg m−3\rho_m = 3300\,\mathrm{kg}\,\mathrm{m}^{-3} and ρw=1000 kg m−3\rho_w = 1000\,\mathrm{kg}\,\mathrm{m}^{-3}, and time counted in millions of years (κ×1 Myr=5618 m\sqrt{\kappa\times1\,\mathrm{Myr}} = 5618\,\mathrm{m}), the theorem gives C=393 m Myr−1/2C = 393\,\mathrm{m}\,\mathrm{Myr}^{-1/2}. The constants fitted by Parsons and Sclater to the depths of the North Pacific and the North Atlantic, once the sediments are removed, are close: dr≈2500 md_r \approx 2500\,\mathrm{m} and C≈350 m Myr−1/2C \approx 350\,\mathrm{m}\,\mathrm{Myr}^{-1/2}, from 0 to 70 Myr70\,\mathrm{Myr}. The values of α\alpha and TmT_m used above are those of their plate model for old floor, a mantle at 1350∘C1350{}^{\circ}\mathrm{C} and α=3.2×10−5 /∘C\alpha = 3.2 \times 10^{-5}\,/{}^{\circ}\mathrm{C}, uncertain by a fifth and a third respectively, so that the agreement of 393 with 350 is as good as could be hoped.

Example 13.8 (Ocean floor 25 and 100 million years old)

With d=2500+350td = 2500 + 350\sqrt t (metres, tt in millions of years), floor 25 Myr25\,\mathrm{Myr} old lies at 2500+350×5=4250 m2500 + 350\times5 = 4250\,\mathrm{m} and floor 100 Myr100\,\mathrm{Myr} old at 2500+350×10=6000 m2500 + 350\times10 = 6000\,\mathrm{m}. The floor sinks 1750 m1750\,\mathrm{m} in its first 25 million years, and only 1750 m1750\,\mathrm{m} more in the next 75.

Depth of the ocean floor against the square root of its age. Each point is the median depth of the one-degree cells of the world ocean whose floor falls in a two-million-year age bin (31 538 cells, deeper than 1000\, m); the grey band holds the middle half of them. The half-space law is a straight line in this plot. Young floor follows it closely; older floor lies above it, because the cells carry their sediments and include seamounts and volcanic plateaus, and because old floor stops sinking (dashed: the plate model). Data: ETOPO1 (NOAA) and the ocean-floor ages of Seton and others (2020).
Depth of the ocean floor against the square root of its age. Each point is the median depth of the one-degree cells of the world ocean whose floor falls in a two-million-year age bin (31 538 cells, deeper than 1000 m1000\,\mathrm{m}); the grey band holds the middle half of them. The half-space law is a straight line in this plot. Young floor follows it closely; older floor lies above it, because the cells carry their sediments and include seamounts and volcanic plateaus, and because old floor stops sinking (dashed: the plate model). Data: ETOPO1 (NOAA) and the ocean-floor ages of Seton and others (2020).

The figure tests the theorem on the whole ocean. Up to about 20 Myr20\,\mathrm{Myr} (t≈4.5\sqrt t \approx 4.5) the medians lie within about a hundred metres of the law. A straight line fitted to the medians younger than 70 Myr70\,\mathrm{Myr} has a slope of only 250 m Myr−1/2250\,\mathrm{m}\,\mathrm{Myr}^{-1/2}: the measured depths are those of the sediment surface, while the law gives the depth of the top of the crust, and the sediment cover thickens with age. Between 60 and 80 Myr80\,\mathrm{Myr}, the floor departs from the square-root law even after its sediments are removed: it becomes shallower than the law, and stops sinking. The plate model, a plate 125 km125\,\mathrm{km} thick whose base is held at the mantle temperature, describes this flattening: its depth tends to about 6400 m6400\,\mathrm{m}, and its heat flow to a constant, as if heat were supplied to the base of old plates by the convecting mantle. That model is studied in the Year 3 volume; in this book the square-root law is used up to 80 Myr80\,\mathrm{Myr}.

Method 13.9 (Dating ocean floor from its depth)

To estimate the age of ocean floor where its magnetic anomalies are absent or unmapped:

  1. measure the depth of the floor and, from seismic profiles, the thickness of its sediments; take the depth dd of the top of the crust, corrected for the weight of the sediments;
  2. invert the law: t=((d−dr)/C)2t = \bigl((d - d_r)/C\bigr)^2, with drd_r and CC for the ocean concerned;
  3. check that the floor is younger than about 80 Myr80\,\mathrm{Myr}, and estimate the uncertainty: an error δd\delta d on the depth gives δt=2t δd/(d−dr)\delta t = 2t\,\delta d/(d - d_r).

For floor at 4600 m4600\,\mathrm{m}, t=(2100/350)2=36 Myrt = (2100/350)^2 = 36\,\mathrm{Myr}, and an uncertainty of 100 m100\,\mathrm{m} on the depth gives 2×36×100/2100≈3.4 Myr2\times36\times100/2100 \approx 3.4\,\mathrm{Myr} on the age. Where floor is shallower than the law predicts over a broad region, a swell, the cause is not age but heat from below (Chapter 15).

The law also links the ocean to the sea level. A ridge that spreads faster carries young, shallow floor farther from its axis; the ocean basins hold less water, and the sea rises over the continents. Over tens of millions of years, changes in spreading rate are one of the two main causes of the changes of global sea level, with the volume of ice on land.

13.5 Transform faults and fracture zones

Ridges are not continuous lines: they are cut into segments offset by faults that run at right angles to them, along the direction of spreading. Beyond the offsets, the faults continue as long scars across the ocean floor.

Definition 13.10 (Transform fault, fracture zone)

A transform fault is a strike-slip fault that is a plate boundary and ends at other plate boundaries; a ridge–ridge transform links the ends of two offset ridge segments. A fracture zone is the continuation of a transform fault beyond the ends of the ridge segments: a linear valley or step across the ocean floor separating floor of different ages that belongs to a single plate.

Proposition 13.11 (Slip on a ridge–ridge transform)

Two ridge segments spreading symmetrically at the half rate uu, perpendicular to themselves, are offset by a transform fault of length aa. Then:

  1. the two sides of the transform slip past each other at the full rate 2u2u, in the sense opposite to the one the offset would suggest if a single straight ridge had been cut and displaced by the fault;
  2. along the fracture zones the two sides do not move relative to each other, and the floor on the two sides differs in age by a/ua/u;
  3. the length of the transform does not change with time.

Proof. Take the xx axis along the transform, towards the east, and the yy axis towards the north, in the frame of the ridge. Let the northern segment lie on x=0x = 0, y>0y > 0, and the southern one on x=ax = a, y<0y < 0 (the offset is to the east going south); the transform is the segment 0<x<a0 < x < a of y=0y = 0. The western plate WW lies west of both segments and moves at −u-u along xx; the eastern plate EE lies east of both and moves at +u+u.

(1) Just north of the transform, at 0<x<a0 < x < a, the floor lies east of the northern segment: it belongs to EE and moves east at uu. Just south of it, the floor lies west of the southern segment: it belongs to WW and moves west at uu. The northern side moves east at 2u2u relative to the southern side: seen from either side, the far side moves to the right, and the slip is right-lateral (dextral). A straight ridge cut by the fault, its southern part now east of its northern part, would instead record a left-lateral (sinistral) displacement.

(2) For x>ax > a, both sides lie east of their segments and belong to EE: they move together. At the distance xx from the northern segment, floor north of the fracture zone has the age x/ux/u; floor south of it is at x−ax - a from the southern segment and has the age (x−a)/u(x - a)/u. The difference is a/ua/u. The same holds for x<0x < 0, where both sides belong to WW.

(3) Both segments stay at x=0x = 0 and x=ax = a in the frame of the ridge, since each spreads symmetrically: the transform keeps the length aa. ∎

J. Tuzo Wilson saw in 1965 that offsets of ridges cannot be read as the displacement of an older, straight ridge, and predicted the sense of slip of the proposition; the focal mechanisms of earthquakes on transforms confirmed it. Earthquakes occur along the active transform, between the ridge ends; the fracture zones are usually quiet. Across a fracture zone the floor of the two sides has different ages, hence, by the depth–age law, different depths: a step that fades slowly with distance from the ridge. In the North Atlantic near 52∘52{}^{\circ} N, the two Charlie–Gibbs transforms offset the Mid-Atlantic Ridge by about 350 km350\,\mathrm{km} in all.

A ridge offset by a transform fault, in map view, north up. The two plates move apart from each segment (black arrows); along the transform (red) they slide past each other right-laterally (half-arrows), although the offset of the ridge looks left-lateral. Grey lines are isochrons, labelled in millions of years: across each fracture zone (dashed) floor of different ages, hence different depths, lies side by side, but both sides move together. Stars: earthquakes, confined to the transform.
A ridge offset by a transform fault, in map view, north up. The two plates move apart from each segment (black arrows); along the transform (red) they slide past each other right-laterally (half-arrows), although the offset of the ridge looks left-lateral. Grey lines are isochrons, labelled in millions of years: across each fracture zone (dashed) floor of different ages, hence different depths, lies side by side, but both sides move together. Stars: earthquakes, confined to the transform.

Transforms are the third kind of evidence for the plate motions of Chapter 12: a transform runs along the relative velocity of the two plates, so it lies on a small circle about their Euler pole, and the great circles drawn perpendicular to several transforms meet at the pole. Fracture zones, traced across the ocean floor, record the direction of motion in the past, as the magnetic anomalies record its rate.

13.6 Exercises

Exercise 13.1 ★

In 2005 a segment of the Afar rift 60 km60\,\mathrm{km} long opened by up to 8 m8\,\mathrm{m}, and 2.5 km32.5\,\mathrm{km}^{3} of magma was intruded. (a) If the dyke had been 8 m8\,\mathrm{m} thick along the whole segment, what would its mean height have been? (b) At the plate rate of 18 mm yr−118\,\mathrm{mm}\,\mathrm{yr}^{-1}, how many years of motion does an opening of 8 m8\,\mathrm{m} represent?

Solution

Solution of Exercise 13.1.

(a) The dyke would cover 60 000 m×8 m=4.8×105 m260\,000\,\mathrm{m}\times8\,\mathrm{m} = 4.8 \times 10^{5}\,\mathrm{m}^{2} in plan, so its mean height would be 2.5×109 m3/4.8×105 m2=5200 m2.5 \times 10^{9}\,\mathrm{m}^{3}/4.8 \times 10^{5}\,\mathrm{m}^{2} = 5200\,\mathrm{m}, about 5 km5\,\mathrm{km}: the dyke cut through much of the crust. (b) 8 m/0.018 m yr−1=4448\,\mathrm{m}/0.018\,\mathrm{m}\,\mathrm{yr}^{-1} = 444 years, some four centuries.

Exercise 13.2 ★

A half-graben is bounded by a border fault of throw 3.0 km3.0\,\mathrm{km} dipping 60∘60{}^{\circ}, and cut by a smaller antithetic fault of throw 0.8 km0.8\,\mathrm{km} dipping 70∘70{}^{\circ}. (a) Compute the heave of each fault and the extension of the section. (b) The section is now 25 km25\,\mathrm{km} wide: how wide was it before the faulting?

Solution

Solution of Exercise 13.2.

(a) The heave is the throw divided by the tangent of the dip: 3.0/tan⁡60∘=1.73 km3.0/\tan60{}^{\circ} = 1.73\,\mathrm{km} and 0.8/tan⁡70∘=0.29 km0.8/\tan70{}^{\circ} = 0.29\,\mathrm{km}; the extension of the section is 2.02 km2.02\,\mathrm{km}. (b) Before the faulting the section was 25−2.02=22.98 km25 - 2.02 = 22.98\,\mathrm{km} wide, about 23 km23\,\mathrm{km}: it has been lengthened by about 9 %9\,\%.

Exercise 13.3 ★

Class the following ridges with the limits of the definition, from their full spreading rates computed with plate vectors: Gakkel Ridge 12 mm yr−112\,\mathrm{mm}\,\mathrm{yr}^{-1}; central Red Sea 15 mm yr−115\,\mathrm{mm}\,\mathrm{yr}^{-1}; Reykjanes Ridge 19 mm yr−119\,\mathrm{mm}\,\mathrm{yr}^{-1}; western Carlsberg Ridge 23 mm yr−123\,\mathrm{mm}\,\mathrm{yr}^{-1}; South Atlantic at 20∘20{}^{\circ} S 33 mm yr−133\,\mathrm{mm}\,\mathrm{yr}^{-1}; East Pacific Rise at 20∘20{}^{\circ} S 143 mm yr−1143\,\mathrm{mm}\,\mathrm{yr}^{-1}. Which of them would you expect to have an axial valley, and which an axial high?

Solution

Solution of Exercise 13.3.

Ultraslow (below 20 mm yr−120\,\mathrm{mm}\,\mathrm{yr}^{-1}): the Gakkel Ridge (12), the central Red Sea (15) and the Reykjanes Ridge (19), the last close to the limit. Slow (20 to 55 mm yr−155\,\mathrm{mm}\,\mathrm{yr}^{-1}): the western Carlsberg Ridge (23) and the South Atlantic (33). Fast (above 75 mm yr−175\,\mathrm{mm}\,\mathrm{yr}^{-1}): the East Pacific Rise (143). The ultraslow and slow ridges should have an axial valley between normal faults; the East Pacific Rise an axial high.

Exercise 13.4 ★

About 3.0 km23.0\,\mathrm{km}^{2} of new ocean floor is made each year, with a crust 7.1 km7.1\,\mathrm{km} thick. (a) What volume of crust is made each year? (b) At this rate, how long would it take to make the 3.028×108 km23.028 \times 10^{8}\,\mathrm{km}^{2} of the ocean floor? Compare with the age of the oldest ocean floor, about 190 Myr190\,\mathrm{Myr}, and explain why the two need not agree.

Solution

Solution of Exercise 13.4.

(a) 3.0 km2×7.1 km=21.3 km33.0\,\mathrm{km}^{2}\times7.1\,\mathrm{km} = 21.3\,\mathrm{km}^{3}, about 21 km321\,\mathrm{km}^{3} a year. (b) 3.028×108 km2/3.0 km2 yr−1=1.01×108 yr3.028 \times 10^{8}\,\mathrm{km}^{2}/3.0\,\mathrm{km}^{2}\,\mathrm{yr}^{-1} = 1.01 \times 10^{8}\,\mathrm{yr}, 101 Myr101\,\mathrm{Myr}. The oldest floor, about 190 Myr190\,\mathrm{Myr}, is older because the floor is not destroyed in order of age: subduction consumes floor of every age, some old floor survives where no trench has reached it, and the rate of production has varied.

Exercise 13.5 ★★

With d=2500+350td = 2500 + 350\sqrt t (metres, tt in millions of years): (a) compute the depth of floor 4, 36 and 64 million years old; (b) find the age of floor lying at 4600 m4600\,\mathrm{m} and at 5300 m5300\,\mathrm{m}; (c) by how much does the floor sink between 4 and 36 Myr36\,\mathrm{Myr}, and between 36 and 64 Myr64\,\mathrm{Myr}?

Solution

Solution of Exercise 13.5.

(a) 2500+350×2=3200 m2500 + 350\times2 = 3200\,\mathrm{m}, 2500+350×6=4600 m2500 + 350\times6 = 4600\,\mathrm{m}, 2500+350×8=5300 m2500 + 350\times8 = 5300\,\mathrm{m}. (b) t=((d−2500)/350)2t = \bigl((d - 2500)/350\bigr)^2: (2100/350)2=36 Myr(2100/350)^2 = 36\,\mathrm{Myr} and (2800/350)2=64 Myr(2800/350)^2 = 64\,\mathrm{Myr}. (c) The floor sinks 1400 m1400\,\mathrm{m} between 4 and 36 Myr36\,\mathrm{Myr}, but only 700 m700\,\mathrm{m} between 36 and 64 Myr64\,\mathrm{Myr}, over a similar length of time.

Exercise 13.6 ★★

Compute the constant CC of the depth–age law (Theorem 13.7) for α=3.2×10−5 K−1\alpha = 3.2 \times 10^{-5}\,\mathrm{K}^{-1}, ρm=3300 kg m−3\rho_m = 3300\,\mathrm{kg}\,\mathrm{m}^{-3}, ρw=1000 kg m−3\rho_w = 1000\,\mathrm{kg}\,\mathrm{m}^{-3}, Tm−T0=1350 KT_m - T_0 = 1350\,\mathrm{K} and κ=10−6 m2 s−1\kappa = 10^{-6}\,\mathrm{m}^{2}\,\mathrm{s}^{-1}, in m Myr−1/2\mathrm{m}\,\mathrm{Myr}^{-1/2}. Redo it for a mantle 250 K250\,\mathrm{K} colder. Which constant would the floor of a colder ocean follow?

Solution

Solution of Exercise 13.6.

The effective expansion coefficient is 3.2×10−5×3300/2300=4.591×10−5 K−13.2 \times 10^{-5}\times3300/2300 = 4.591 \times 10^{-5}\,\mathrm{K}^{-1}, and κ×1 Myr=10−6×3.156×1013=5618 m\sqrt{\kappa\times1\,\mathrm{Myr}} = \sqrt{10^{-6}\times3.156 \times 10^{13}} = 5618\,\mathrm{m}. Then C=(2/π)×4.591×10−5×1350×5618=1.1284×4.591×10−5×1350×5618=393 m Myr−1/2C = (2/\sqrt\pi)\times4.591 \times 10^{-5}\times1350\times5618 = 1.1284\times4.591 \times 10^{-5}\times1350\times5618 = 393\,\mathrm{m}\,\mathrm{Myr}^{-1/2}. For a mantle 250 K250\,\mathrm{K} colder, CC scales with Tm−T0T_m - T_0: 393×1100/1350=320 m Myr−1/2393\times1100/1350 = 320\,\mathrm{m}\,\mathrm{Myr}^{-1/2}. The floor of a colder ocean sinks more slowly and follows the smaller constant. The fitted 350350 of the chapter is not such a case: it lies within the uncertainty of the parameters.

Exercise 13.7 ★★

The plate model gives the heat flow of the ocean floor as q=11.3/tq = 11.3/\sqrt t, in units of 10−6 cal cm−2 s−110^{-6}\,\mathrm{cal}\,\mathrm{cm}^{-2}\,\mathrm{s}^{-1}, with tt in millions of years. (a) Convert the constant to mW m−2 Myr1/2\mathrm{mW}\,\mathrm{m}^{-2}\,\mathrm{Myr}^{1/2} (1 cal=4.184 J1\,\mathrm{cal} = 4.184\,\mathrm{J}) and compare it with the 490 mW m−2 Myr1/2490\,\mathrm{mW}\,\mathrm{m}^{-2}\,\mathrm{Myr}^{1/2} of Chapter 10. (b) Compute qq at 1, 10 and 150 Myr150\,\mathrm{Myr}. The law was fitted to floor up to 120 Myr120\,\mathrm{Myr} old, and the plate model makes the heat flow of older floor level off at a constant: is the value at 150 Myr150\,\mathrm{Myr} then too high or too low?

Solution

Solution of Exercise 13.7.

(a) 10−6 cal cm−2 s−1=4.184×10−6×104=4.184×10−2 W m−2=41.84 mW m−210^{-6}\,\mathrm{cal}\,\mathrm{cm}^{-2}\,\mathrm{s}^{-1} = 4.184 \times 10^{-6}\times10^{4} = 4.184 \times 10^{-2}\,\mathrm{W}\,\mathrm{m}^{-2} = 41.84\,\mathrm{mW}\,\mathrm{m}^{-2}, so the constant is 11.3×41.84=473 mW m−2 Myr1/211.3\times41.84 = 473\,\mathrm{mW}\,\mathrm{m}^{-2}\,\mathrm{Myr}^{1/2}, 3.5 %3.5\,\% below the 490 of Chapter 10: the two fits agree. (b) q=473q = 473, 473/10=150473/\sqrt{10} = 150 and 473/150=38.6 mW m−2473/\sqrt{150} = 38.6\,\mathrm{mW}\,\mathrm{m}^{-2}. The square-root law keeps falling, while the plate model levels off at a constant: at 150 Myr150\,\mathrm{Myr} the square-root value is too low, as the depth law goes too deep.

Exercise 13.8 ★★

A ridge trending north–south is cut into two segments; going south along the ridge, the axis jumps 40 km40\,\mathrm{km} to the west at a transform fault. (a) What is the sense of slip on the transform? (b) What does the offset of the ridge seem to show? (c) Where along the line of the transform do earthquakes occur, and why not beyond?

Solution

Solution of Exercise 13.8.

Take the northern segment on x=0x = 0 and the southern one on x=−40x = -40 (km), the transform on y=0y = 0 between them. (a) Just north of the transform the floor lies west of the northern segment and moves west; just south of it, it lies east of the southern segment and moves east. Seen from either side, the far side moves to the left: the slip is left-lateral (sinistral). (b) The ridge seems to have been displaced right-laterally, its southern part to the west: the opposite sense, as Proposition 13.11 predicts. (c) Earthquakes occur only on the 40 km40\,\mathrm{km} between the two ridge ends, where the two sides belong to different plates; beyond, along the fracture zones, both sides belong to the same plate and move together.

Exercise 13.9 ★★

The Charlie–Gibbs fracture zones offset the Mid-Atlantic Ridge by 350 km350\,\mathrm{km} in all; the full spreading rate there is 21.2 mm yr−121.2\,\mathrm{mm}\,\mathrm{yr}^{-1}. Treat the offset as a single transform. (a) What is the difference in age across the fracture zone? (b) Using d=2500+350td = 2500 + 350\sqrt t, compute the depth step across the fracture zone at the end of the transform, then 100 km100\,\mathrm{km} and 1000 km1000\,\mathrm{km} beyond it.

Solution

Solution of Exercise 13.9.

The half rate is 10.6 mm yr−110.6\,\mathrm{mm}\,\mathrm{yr}^{-1}, 10.6 km Myr−110.6\,\mathrm{km}\,\mathrm{Myr}^{-1}. (a) The age step is 350/10.6=33.0 Myr350/10.6 = 33.0\,\mathrm{Myr}. (b) At the end of the transform, floor 33.0 Myr33.0\,\mathrm{Myr} old (2500+35033.0=4511 m2500 + 350\sqrt{33.0} = 4511\,\mathrm{m}) faces floor of age 0 (2500 m2500\,\mathrm{m}): a step of about 2010 m2010\,\mathrm{m}. 100 km100\,\mathrm{km} beyond, the ages are 450/10.6=42.5450/10.6 = 42.5 and 100/10.6=9.4 Myr100/10.6 = 9.4\,\mathrm{Myr}, the depths 4781 and 3575 m3575\,\mathrm{m}: a step of about 1210 m1210\,\mathrm{m}. 1000 km1000\,\mathrm{km} beyond, the ages are 127.4 and 94.3 Myr94.3\,\mathrm{Myr}, the depths 6450 and 5899 m5899\,\mathrm{m}: 550 m550\,\mathrm{m}. (These ages are beyond 80 Myr80\,\mathrm{Myr}, where the square-root law goes too deep; the plate law would give a smaller step.)

Exercise 13.10 ★★★

An ocean basin is made at a constant rate and holds floor of every age from 0 to AA in equal areas. (a) Show that its mean depth is dr+23CAd_r + \frac23C\sqrt A. (b) With dr=2500 md_r = 2500\,\mathrm{m} and C=350 m Myr−1/2C = 350\,\mathrm{m}\,\mathrm{Myr}^{-1/2}, compare A=180 MyrA = 180\,\mathrm{Myr} and A=120 MyrA = 120\,\mathrm{Myr}. (c) If the spreading of the basin speeds up so that its oldest floor is 120 Myr120\,\mathrm{Myr} instead of 180 Myr180\,\mathrm{Myr}, by how much does sea level rise, neglecting the flooding of the continents but allowing for the load of the extra water on the floor, which sinks by ρw/(ρm−ρw)\rho_w/(\rho_m - \rho_w) times the rise (ρm=3300\rho_m = 3300, ρw=1000 kg m−3\rho_w = 1000\,\mathrm{kg}\,\mathrm{m}^{-3})?

Solution

Solution of Exercise 13.10.

(a) With equal areas for every age, the mean depth is the mean of d(t)d(t) over [0,A][0, A]:

1A∫0A(dr+Ct)dt=dr+CA⋅23A3/2=dr+23CA.\frac1A\int_0^A\bigl(d_r + C\sqrt t\bigr)\mathrm dt = d_r + \frac CA\cdot\frac23A^{3/2} = d_r + \frac23C\sqrt A.

(b) For A=180 MyrA = 180\,\mathrm{Myr}: 2500+23×350×13.416=5630 m2500 + \frac23\times350\times13.416 = 5630\,\mathrm{m}; for 120 Myr120\,\mathrm{Myr}: 2500+23×350×10.954=5056 m2500 + \frac23\times350\times10.954 = 5056\,\mathrm{m}, 574 m574\,\mathrm{m} shallower. (c) Let the sea rise by rr and the loaded floor sink by s=rρw/(ρm−ρw)s = r\rho_w/(\rho_m - \rho_w). The water, unchanged in volume, must fill the same depth over the same area, so r+s=574 mr + s = 574\,\mathrm{m}, r ρm/(ρm−ρw)=574r\,\rho_m/(\rho_m - \rho_w) = 574, and r=574×2300/3300=400 mr = 574\times2300/3300 = 400\,\mathrm{m}: hundreds of metres, from the spreading rate alone.

Exercise 13.11 ★★★

In the setting of Proposition 13.11, the depth step across a fracture zone at the distance x>ax > a from the farther ridge segment is Δd=C(x/u−(x−a)/u)\Delta d = C\bigl(\sqrt{x/u} - \sqrt{(x - a)/u}\bigr). (a) Show that, for x≫ax \gg a, Δd≈Ca/(2ux)\Delta d \approx Ca/(2\sqrt{ux}). (b) With C=350 m Myr−1/2C = 350\,\mathrm{m}\,\mathrm{Myr}^{-1/2}, a=350 kma = 350\,\mathrm{km} and u=10.6 km Myr−1u = 10.6\,\mathrm{km}\,\mathrm{Myr}^{-1}, compare the exact and approximate steps at x=450x = 450, 1350 and 3350 km3350\,\mathrm{km}. When is the approximation good to 10 %10\,\%?

Solution

Solution of Exercise 13.11.

(a) x−a=x1−a/x≈x (1−a/2x)\sqrt{x - a} = \sqrt x\sqrt{1 - a/x} \approx \sqrt x\,(1 - a/2x) for a≪xa \ll x, so Δd≈Cx/u⋅a/(2x)=Ca/(2ux)\Delta d \approx C\sqrt{x/u}\cdot a/(2x) = Ca/(2\sqrt{ux}). (b) At x=450 kmx = 450\,\mathrm{km}: exact 1205 m1205\,\mathrm{m}, approximate 350×350/(210.6×450)=887 m350\times350/(2\sqrt{10.6\times450}) = 887\,\mathrm{m}; at 1350 km1350\,\mathrm{km}: 550 m550\,\mathrm{m} and 512 m512\,\mathrm{m}; at 3350 km3350\,\mathrm{km}: 334 m334\,\mathrm{m} and 325 m325\,\mathrm{m}. The ratio of the approximate to the exact step depends only on r=a/xr = a/x: (r/2)/(1−1−r)(r/2)/(1 - \sqrt{1 - r}), which is 0.9 for r=0.36r = 0.36. The approximation is good to 10 %10\,\% beyond x=350/0.36≈970 kmx = 350/0.36 \approx 970\,\mathrm{km}, about three offsets from the ridge.

Exercise 13.12 ★★★

Compare the half-space law d1(t)=2500+350td_1(t) = 2500 + 350\sqrt t with the plate law d2(t)=6400−3200 e−t/62.8d_2(t) = 6400 - 3200\,e^{-t/62.8}. (a) Compute d2−d1d_2 - d_1 at 10, 20, 30 and 40 Myr40\,\mathrm{Myr}. (b) Show that the two laws are equal at one age between 20 and 30 Myr30\,\mathrm{Myr} and find it to 0.1 Myr0.1\,\mathrm{Myr} by bisection. (c) Compare their slopes there. Why may the two laws be joined at that age without a visible break?

Solution

Solution of Exercise 13.12.

(a) d2−d1=3671.1−3606.8=64.3 md_2 - d_1 = 3671.1 - 3606.8 = 64.3\,\mathrm{m} at 10 Myr10\,\mathrm{Myr}; 4072.8−4065.3=7.5 m4072.8 - 4065.3 = 7.5\,\mathrm{m} at 20; 4415.4−4417.0=−1.7 m4415.4 - 4417.0 = -1.7\,\mathrm{m} at 30; 4707.5−4713.6=−6.1 m4707.5 - 4713.6 = -6.1\,\mathrm{m} at 40. (b) d2−d1d_2 - d_1 is positive at 20 and negative at 30, and both laws are continuous: they are equal in between. Bisection: at 25, d2−d1=+0.9d_2 - d_1 = +0.9; at 27.5, −0.7-0.7; at 26.25, +0.01+0.01; at 26.875, −0.3-0.3; at 26.56, −0.2-0.2; at 26.41, −0.08-0.08; at 26.33, −0.04-0.04: the root lies between 26.25 and 26.33, at 26.3 Myr26.3\,\mathrm{Myr}, where both give 4294 m4294\,\mathrm{m}. (c) d1′=175/26.3=34.1 m Myr−1d_1' = 175/\sqrt{26.3} = 34.1\,\mathrm{m}\,\mathrm{Myr}^{-1} and d2′=(3200/62.8) e−26.3/62.8=33.5 m Myr−1d_2' = (3200/62.8)\,e^{-26.3/62.8} = 33.5\,\mathrm{m}\,\mathrm{Myr}^{-1}. The laws have nearly the same value and the same slope there, so the joined curve has no visible kink.

13.7 Problem: The birth of an ocean

Problem 13.1

Weekend problem — a continent stretched by its faults, a young ocean measured by its stripes, and the depth of its floor as it ages

Take R=6371 kmR = 6371\,\mathrm{km}. An ocean is born in three stages, each seen today in a different place: a continental rift, a young ocean, an old ocean.

Part I — A rift stretched by its faults. A section across a rift trending 020∘020{}^{\circ} crosses six normal faults whose throws and dips were measured on seismic profiles:

faultF1F2F3F4F5F6
throw (m\mathrm{m})600110024003508001500
dip60∘60{}^{\circ}55∘55{}^{\circ}50∘50{}^{\circ}65∘65{}^{\circ}60∘60{}^{\circ}52∘52{}^{\circ}

The faults cut lavas dated 3.2 Ma3.2\,\mathrm{Ma}, and the rift is now 60 km60\,\mathrm{km} wide.

  1. Compute the heave of each fault. Which is the border fault?
  2. Compute the extension of the section, and the width of the rift before the faulting.
  3. The two plates separate at 6.0 mm yr−16.0\,\mathrm{mm}\,\mathrm{yr}^{-1} towards 105∘105{}^{\circ}. Compute the component of this motion perpendicular to the rift.
  4. How long would the plates take to produce the extension of question 2?
  5. How much have the plates moved apart since the lavas were erupted? What fraction of it do the faults carry?
  6. Suggest where the rest of the extension has gone. If it were taken up by dykes like that of Afar in 2005, 8 m8\,\mathrm{m} wide, how many would be needed, and how often?

Part II — A young ocean measured by its stripes. A magnetic profile across the axis of the central Red Sea, at 18.0∘18.0{}^{\circ} N, 40.0∘40.0{}^{\circ} E, runs along the direction of spreading. The young edge of chron C2An (2.581 Ma2.581\,\mathrm{Ma}) lies 21.0 km21.0\,\mathrm{km} north-east of the axis and 20.2 km20.2\,\mathrm{km} south-west of it; the old edge of chron C3n (5.235 Ma5.235\,\mathrm{Ma}) lies at 41.0 km41.0\,\mathrm{km} and 40.2 km40.2\,\mathrm{km}. The edges of anomalies are displaced outward from the axis by 2.2 km2.2\,\mathrm{km} in all, on average, over both flanks.

  1. Compute the full spreading rate from each chron, without correction.
  2. Correct each rate for the outward displacement. Do the two agree?
  3. Show that the rate computed from the distance between the two chrons on each flank needs no correction, and compute it.
  4. Compute the half rates on each flank from the distances between the two chrons. Is the spreading symmetric?
  5. The Euler pole of Arabia relative to Nubia is at 30.9∘30.9{}^{\circ} N, 23.6∘23.6{}^{\circ} E, with the rate 0.403∘/Myr0.403{}^{\circ}/\mathrm{Myr}. Compute the angular distance from the pole to the profile, and the full spreading rate the plate vector predicts there.
  6. In the northern Red Sea, at 26.0∘26.0{}^{\circ} N, 35.0∘35.0{}^{\circ} E, compute the angular distance from the pole and the predicted rate.
  7. Compare these rates with those measured, 15 and 9 mm yr−19\,\mathrm{mm}\,\mathrm{yr}^{-1}. Why does the Red Sea open faster in the south?

Part III — Towards an Atlantic.

  1. How wide is the oceanic floor made in the central Red Sea since the old edge of C3n, at the rate of question 9?
  2. The South Atlantic opened by about 5000 km5000\,\mathrm{km} at Recife in 120.6 Myr120.6\,\mathrm{Myr} (Chapter 12). Compute its mean rate of opening.
  3. At the present rate of the central Red Sea, how long would an opening of 5000 km5000\,\mathrm{km} take? And at the rate of the northern Red Sea?
  4. The Red Sea opens about a pole close to it. What does this imply for its shape as it widens, and for the time the northern part needs to reach the width the central part has now?
  5. Which kind of ridge is the Red Sea axis, and which form of axis do you expect?

Part IV — The floor sinks. Use d=2500+350td = 2500 + 350\sqrt t (metres, tt in millions of years) and, for comparison, the plate law 6400−3200 e−t/62.86400 - 3200\,e^{-t/62.8}.

  1. Compute the depth of the new floor at the ages of 1, 10 and 40 Myr40\,\mathrm{Myr}.
  2. At what age does the floor reach 4000 m4000\,\mathrm{m}?
  3. The floor next to each passive margin is as old as the ocean. By how much does it sink in the first 10 Myr10\,\mathrm{Myr} after break-up, and between 70 and 80 Myr80\,\mathrm{Myr}?
  4. At what rate, in metres per million years, is that floor sinking when the ocean is 80 Myr80\,\mathrm{Myr} old?
  5. What heat flow does the floor of question 22 lose then, with q=490/tq = 490/\sqrt t in mW m−2\mathrm{mW}\,\mathrm{m}^{-2}?
  6. Compute the depth of floor 80 Myr80\,\mathrm{Myr} old with each of the two laws, and their difference. Why may the two be compared at this age?
  7. To the nearest tenth of a kilometre, how deep does the square-root law put the sea floor of the new ocean when it is 80 million years old?
Solution

Solution of Problem 13.1.

1. Heave == throw/tan⁡/\tan(dip): F1 346 m346\,\mathrm{m}, F2 770 m770\,\mathrm{m}, F3 2014 m2014\,\mathrm{m}, F4 163 m163\,\mathrm{m}, F5 462 m462\,\mathrm{m}, F6 1172 m1172\,\mathrm{m}. F3, with the largest throw and heave, is the border fault.

2. The extension is the sum, 4927 m4927\,\mathrm{m}, about 4.9 km4.9\,\mathrm{km}. The rift was 60−4.9=55.1 km60 - 4.9 = 55.1\,\mathrm{km} wide before the faulting.

3. The normal to a rift trending 020∘020{}^{\circ} points to 110∘110{}^{\circ}; the motion, towards 105∘105{}^{\circ}, makes 5∘5{}^{\circ} with it. The perpendicular component is 6.0cos⁡5∘=5.98 mm yr−16.0\cos5{}^{\circ} = 5.98\,\mathrm{mm}\,\mathrm{yr}^{-1}.

4. 4.927 km/5.98 km Myr−1=0.82 Myr4.927\,\mathrm{km}/5.98\,\mathrm{km}\,\mathrm{Myr}^{-1} = 0.82\,\mathrm{Myr}.

5. In 3.2 Myr3.2\,\mathrm{Myr} the plates moved apart by 5.98×3.2=19.1 km5.98\times3.2 = 19.1\,\mathrm{km} across the rift. The faults carry 4.93/19.1=26 %4.93/19.1 = 26\,\% of it.

6. The other three quarters, 14.2 km14.2\,\mathrm{km}, are not in the faults of the section. They may be taken up by dykes intruded along the axis, which open the rift without faulting it, as in Afar, or by faults outside the section. With dykes 8 m8\,\mathrm{m} wide, 14 200 m/8 m≈178014\,200\,\mathrm{m}/8\,\mathrm{m} \approx 1780 dykes are needed, one every 3.2×106/1780≈18003.2\times10^6/1780 \approx 1800 years on average.

7. From C2An: (21.0+20.2)/2.581=41.2/2.581=15.96 mm yr−1(21.0 + 20.2)/2.581 = 41.2/2.581 = 15.96\,\mathrm{mm}\,\mathrm{yr}^{-1}. From C3n: (41.0+40.2)/5.235=81.2/5.235=15.51 mm yr−1(41.0 + 40.2)/5.235 = 81.2/5.235 = 15.51\,\mathrm{mm}\,\mathrm{yr}^{-1}.

8. (41.2−2.2)/2.581=15.11 mm yr−1(41.2 - 2.2)/2.581 = 15.11\,\mathrm{mm}\,\mathrm{yr}^{-1} and (81.2−2.2)/5.235=15.09 mm yr−1(81.2 - 2.2)/5.235 = 15.09\,\mathrm{mm}\,\mathrm{yr}^{-1}: corrected, the two agree to 0.02 mm yr−10.02\,\mathrm{mm}\,\mathrm{yr}^{-1}. The correction matters more for the younger chron, whose distance is shorter.

9. The outward displacement shifts both edges of a flank by the same amount, so it cancels in their difference. Over both flanks, (81.2−41.2)/(5.235−2.581)=40.0/2.654=15.07 mm yr−1(81.2 - 41.2)/(5.235 - 2.581) = 40.0/2.654 = 15.07\,\mathrm{mm}\,\mathrm{yr}^{-1}.

10. North-east: (41.0−21.0)/2.654=7.54 mm yr−1(41.0 - 21.0)/2.654 = 7.54\,\mathrm{mm}\,\mathrm{yr}^{-1}; south-west: (40.2−20.2)/2.654=7.54 mm yr−1(40.2 - 20.2)/2.654 = 7.54\,\mathrm{mm}\,\mathrm{yr}^{-1}. The spreading is symmetric; the 0.8 km0.8\,\mathrm{km} difference between the flanks, the same for both chrons, is a constant shift, such as the axis being placed 0.4 km0.4\,\mathrm{km} off centre.

11. cos⁡Δ=sin⁡30.9∘sin⁡18.0∘+cos⁡30.9∘cos⁡18.0∘cos⁡16.4∘=0.15870+0.78287=0.94157\cos\Delta = \sin30.9{}^{\circ}\sin18.0{}^{\circ} + \cos30.9{}^{\circ}\cos18.0{}^{\circ}\cos16.4{}^{\circ} = 0.15870 + 0.78287 = 0.94157, so Δ=19.69∘\Delta = 19.69{}^{\circ}. With ωR=0.403×(π/180)×6371=44.81 mm yr−1\omega R = 0.403\times(\pi/180)\times6371 = 44.81\,\mathrm{mm}\,\mathrm{yr}^{-1}, the rate is 44.81sin⁡19.69∘=15.10 mm yr−144.81\sin19.69{}^{\circ} = 15.10\,\mathrm{mm}\,\mathrm{yr}^{-1}, the corrected rates of questions 8 and 9.

12. cos⁡Δ=sin⁡30.9∘sin⁡26.0∘+cos⁡30.9∘cos⁡26.0∘cos⁡11.4∘=0.22512+0.75600=0.98112\cos\Delta = \sin30.9{}^{\circ}\sin26.0{}^{\circ} + \cos30.9{}^{\circ}\cos26.0{}^{\circ}\cos11.4{}^{\circ} = 0.22512 + 0.75600 = 0.98112, so Δ=11.15∘\Delta = 11.15{}^{\circ} and the rate is 44.81sin⁡11.15∘=8.7 mm yr−144.81\sin11.15{}^{\circ} = 8.7\,\mathrm{mm}\,\mathrm{yr}^{-1}.

13. The predictions, 15.1 and 8.7 mm yr−18.7\,\mathrm{mm}\,\mathrm{yr}^{-1}, match the measured 15 and 9 mm yr−19\,\mathrm{mm}\,\mathrm{yr}^{-1}. The rate is ωRsin⁡Δ\omega R\sin\Delta, and the pole lies north-west of the Red Sea, in north-eastern Libya: the farther south, the farther from the pole, the faster the opening.

14. 15.09×5.235=79 km15.09\times5.235 = 79\,\mathrm{km} of oceanic floor.

15. 5000/120.6=41 km Myr−15000/120.6 = 41\,\mathrm{km}\,\mathrm{Myr}^{-1}, 41 mm yr−141\,\mathrm{mm}\,\mathrm{yr}^{-1} on average.

16. 5000/15.1=331 Myr5000/15.1 = 331\,\mathrm{Myr} at the central rate; 5000/8.7=575 Myr5000/8.7 = 575\,\mathrm{Myr} at the northern rate.

17. Opening about a nearby pole, the Red Sea widens like a pair of scissors: its width grows in proportion to sin⁡Δ\sin\Delta, and it stays a wedge narrowing towards the pole. At 8.7 mm yr−18.7\,\mathrm{mm}\,\mathrm{yr}^{-1}, the northern part needs 79/8.7=9.1 Myr79/8.7 = 9.1\,\mathrm{Myr} to make the 79 km79\,\mathrm{km} of oceanic floor the central part has now.

18. At 15 mm yr−115\,\mathrm{mm}\,\mathrm{yr}^{-1} the Red Sea axis is an ultraslow ridge; an axial valley between normal faults is expected.

19. 2500+350×1=2850 m2500 + 350\times1 = 2850\,\mathrm{m}; 2500+35010=3607 m2500 + 350\sqrt{10} = 3607\,\mathrm{m}; 2500+35040=4714 m2500 + 350\sqrt{40} = 4714\,\mathrm{m}.

20. t=(1500/350)2=18.4 Myrt = (1500/350)^2 = 18.4\,\mathrm{Myr}.

21. In the first 10 Myr10\,\mathrm{Myr} it sinks 35010=1107 m350\sqrt{10} = 1107\,\mathrm{m}; between 70 and 80 Myr80\,\mathrm{Myr}, 350(80−70)=350×(8.944−8.367)=202 m350(\sqrt{80} - \sqrt{70}) = 350\times(8.944 - 8.367) = 202\,\mathrm{m}, five times less over the same time.

22. dd/dt=C/(2t)=175/80=19.6 m Myr−1\mathrm dd/\mathrm dt = C/(2\sqrt t) = 175/\sqrt{80} = 19.6\,\mathrm{m}\,\mathrm{Myr}^{-1}, about 0.02 mm0.02\,\mathrm{mm} a year.

23. 490/80=54.8 mW m−2490/\sqrt{80} = 54.8\,\mathrm{mW}\,\mathrm{m}^{-2}.

24. Square-root law: 2500+35080=2500+350×8.944=5630 m2500 + 350\sqrt{80} = 2500 + 350\times8.944 = 5630\,\mathrm{m}. Plate law: 6400−3200 e−80/62.8=6400−3200×0.2798=5505 m6400 - 3200\,e^{-80/62.8} = 6400 - 3200\times0.2798 = 5505\,\mathrm{m}. They differ by 126 m126\,\mathrm{m}. At 80 Myr80\,\mathrm{Myr} both laws still apply: the square-root law up to about 80 Myr80\,\mathrm{Myr}, the plate law from about 20 Myr20\,\mathrm{Myr}; beyond, the square-root law goes too deep.

25. The square-root law gives 5630 m5630\,\mathrm{m}: to the nearest tenth of a kilometre, the floor of the new ocean lies at a depth of 5.6 km5.6\,\mathrm{km} when it is 80 million years old (the plate law gives 5.5 km5.5\,\mathrm{km}).

本章定义的术语

在术语表中查看全部 957 个术语